A High-Resolution Spectrum of the Extremely Metal-rich Bulge G Dwarf OGLE-2006-BLG-265

@article{Johnson2007AHS,
  title={A High-Resolution Spectrum of the Extremely Metal-rich Bulge G Dwarf OGLE-2006-BLG-265},
  author={Jennifer A. Johnson and Avishay Gal-yam and Douglas C. Leonard and Joshua D. Simon and Andrzej Udalski and Andrew Gould Ohio State and Caltech and San Diego State and Warsaw University Astronomical Observatory},
  journal={The Astrophysical Journal},
  year={2007},
  volume={655}
}
We present an R = 45,000 Keck spectrum of the microlensed Galactic bulge G dwarf OGLE-2006-BLG-265, which has high (~60) signal-to-noise ratio despite its short (15 minute) exposure time, because the source was magnified by A ~ 135. While it is very metal-rich ([Fe/H] = 0.56), the higher temperature of this star compared with the luminous red giants usually measured in the bulge gives its spectrum many unblended atomic lines. We measure the abundances of 17 elements, including the first… 

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